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Simulating X-ray observations of galaxy clusters with the X-ray Integral Field Unit onboard the Athena mission
- Source :
- Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Jun 2018, Austin, United States. pp.162, ⟨10.1117/12.2311957⟩
- Publication Year :
- 2018
- Publisher :
- INTERNATIONAL SOCIETY FOR OPTICAL ENGINEERING, 2018.
-
Abstract
- The X-ray Integral Field Unit (X-IFU) is the cryogenic imaging spectrometer onboard the ESA L2 mission Athena. With its array of almost 3840 superconducting Transition Edge Sensors micro-calorimeters, the X-IFU will provide spatially resolved (5" over the field of view) high-resolution spectroscopy (2.5 eV FWHM up to 7 keV) in the 0.2-12 keV energy band. These transformational capabilities will allow the X-IFU to probe the Hot and Energetic Universe, and notably measure the physical properties of large-scale structures with unprecedented accuracy. Starting from numerically-simulated massive (1014 Mo) galaxy clusters at different steps of their evolution, we investigate the capabilities of the X-IFU in recovering chemical abundances, redshift and gas temperature spatial distributions across time, making use of full field-of-view End-To-End simulations of X-IFU observations. This work serve as feasibility study for the Chemical Enrichment of the Universe science objective. We show that using 100 ks observations, the X-IFU will provide an unprecedented spatially-accurate knowledge of the physics of the ICM (abundances, temperature, bulk-motion). We also demonstrate that challenges related to the data analysis of extended sources with very high-resolution spectrometers (e.g. binning, line of sight mixing, particle background) need to be thoroughly addressed to maximise the science of the instrument.
- Subjects :
- galaxy cluster
chemical enrichment
media_common.quotation_subject
Measure (physics)
Imaging spectrometer
Field of view
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
7. Clean energy
01 natural sciences
010309 optics
0103 physical sciences
galaxy clusters
Athena
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Galaxy cluster
ComputingMilieux_MISCELLANEOUS
media_common
Physics
X-IFU
Line-of-sight
Spectrometer
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
Astrophysics::Instrumentation and Methods for Astrophysics
Universe
Redshift
End-To-End simulations
13. Climate action
End-To-End simulation
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Jun 2018, Austin, United States. pp.162, ⟨10.1117/12.2311957⟩
- Accession number :
- edsair.doi.dedup.....545024318e3a4abc1ffffac8013c9cb1